Semirelativistic Magnetohydrodynamics and Physics-Based Convergence Acceleration

By Tamas I. Gombosi, G. T'oth, D. D. De Zeeuw, K. Hansen, K. Kabin, Kenneth G. Powell. 2002

161 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Computational Mechanics

View Paper: https://www.semanticscholar.org/paper/37629cdbe24ac9a1087257c5123eff2c4553cb4a

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In Astronomy and Astrophysics

1. Matthias Rempel
2. Paul Charbonneau
3. Mark S. Miesch
4. J. Toomre
5. A. Brun
6. M. Browning

In Computational Mechanics

1. Matthias Rempel
2. Paul Charbonneau

Citations in the corpus

• EXTENSION OF THE MURAM RADIATIVE MHD CODE FOR CORONAL SIMULATIONS (2016, methodology): “(1) yields (using xA = vA/c): [ I + x2A(I − b̂b̂) ] % ∂v ∂t = −%(v · ∇)v −∇p+ %g + 1 4π (∇×B)×B (8) The inverse of the “enhanced inertia” matrix on the left hand side is given by (Gombosi et al. 2002)”